Interacting gravitational fields

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SUMMARY

The interaction of gravitational fields is governed by distinct principles in Newtonian gravity and General Relativity (GR). In Newtonian gravity, the equations are linear, allowing for the straightforward addition of individual fields to determine the total gravitational field. Conversely, GR features non-linear equations, necessitating numerical solutions for even simple two-body problems. In weak field environments, such as the solar system, gravitational fields effectively add linearly, but extreme conditions like those near neutron stars and black holes require consideration of non-linear effects.

PREREQUISITES
  • Newtonian gravity principles
  • General Relativity (GR) fundamentals
  • Understanding of gravitational field equations
  • Numerical methods for solving differential equations
NEXT STEPS
  • Study the implications of Newton's law of gravitation
  • Explore the Einstein Field Equations (EFE) in detail
  • Learn about numerical solutions in General Relativity
  • Investigate gravitational effects in extreme environments, such as black holes
USEFUL FOR

Astrophysicists, physicists, and students of gravitational theory seeking to deepen their understanding of gravitational interactions and their implications in various environments.

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How do gravitational fields interact with each other? Because the Earth is in the Sun's and the moon is in the Earth's and the sun's. I think ocean tides on Earth is an example of it, but is there anything more specific? What is happening to an area of space inside multiple gravitational fields?
 
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In Newtonian gravity the equations are linear, so you simply add up the various individual fields to get the total field. In GR the equations are non-linear so you cannot simply add up the various individual field to get the total field. So even a simple two-body problem usually requires a numerical solution in GR.
 
DaleSpam said:
In Newtonian gravity the equations are linear, so you simply add up the various individual fields to get the total field. In GR the equations are non-linear so you cannot simply add up the various individual field to get the total field. So even a simple two-body problem usually requires a numerical solution in GR.

For "weak field" environments like the solar system, fields effectively add linearly for GR as well. For accurate calculations (such as Mercury's perihelion precession) you have to take into account not only the Newtonian field acting on objects at rest but also additional effects caused by motion through curved space, but these additional effects are still proportional to the Newtonian field and still effectively add up linearly for multiple sources.

In practice, you only need to take non-linearity into account in extreme environments such as neutron stars and black holes.
 
But what's happening to the space? If it warps one way, how to it react to warping another way?
 
As I said above, unless you are close to the Newtonian limit, you basically just have to numerically solve the EFE for the situation you have in mind. The nonlinearities make it difficult to make general statements of the kind you are asking.
 
In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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